Asymmetries in asymptotic giant branch stars and their winds - I. From 3D RHD models to synthetic observables

Open Access

Fig. 8.

SEDs from RADMC-3D in six viewing directions as indicated by the sets of angles i and ϕ. Both stellar (gas) and dust data are from st28gm06n052. The legend lists the corresponding integrated flux density of each SED.

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